Modeling proton-induced activation background in high-energy space instrumentation

Authors: Riccardo Campana, Alfonso Pisapia, Lorenzo Amati et al.
Publication: Space Telescopes and Instrumentation 2026: Ultraviolet to Gamma Ray
Published: Aug 21, 2026
Source: Crossref
Back to Search View Original Cite This Article

Related Articles

Quantifying centroid shifts induced by glass in the GFA of JUST

Rui Zhang, Zhen Zhang et al. - Aug 2026

Read More
On-site integration and validation of the SOXS control electronics at ESO-NTT

Mirko Colapietro, Sergio D'Orsi et al. - Aug 2026

Read More
Documented cases of electromagnetic interference in ground-based optical and infrared observatories

Miroslav Vulinovic, Pedro Escárate - Aug 2026

Read More
Project management in support of an innovative engineering approach: the challenge of designing next-generation astronomical instrumentation

Vincenzo Cianniello, Christian Eredia et al. - Aug 2026

Read More
WST instrument exposure time calculator: full simulation of multi-mode spectrograph performance from source to detector

Matteo Ferro, Matteo Genoni et al. - Aug 2026

Read More
Journal Ideas PyMinds Charcha More
PORE

About

About Us

Resources

Help Centre Research Guides CiteScore

Legal

Terms of Service Privacy Policy Cookie Policy Accessibility

Connect

Contact Us
© 2026 PORE. Content available under CC BY-NC 4.0